In terms of AGN feedback, in the case of clusters of galaxies, it is now well established that the buoyantly rising bubbles produced by the activity of the supermassive black hole in the BCG are able to uplift metals in their wake, leading to an abundance enhancement along the axis corresponding to the radio jets compared to the perpendicular direction [1]}, [2]}, [3]}, [4]}. Given the shallower gravitational potential wells of galaxy groups, one might expect this effect to be even more pronounced, and even more important for the physical evolution of the IGrM, as metals produced in the BGG may even escape the group halo through the action of the AGN. However, to our knowledge, a systematic study of the metal asymmetry in groups [3]}, [4]} is still lacking. The main impediment is likely related to the fact that the region of uplift is also generally expected to be multi-phase [1]} which, as discussed in §REF , significantly complicates the determination of an exact Fe budget in a given spatial region.
